Mass, Gas and Galaxies in the Abell 901/902 Supercluster

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Seeing the invisible Meghan Gray (University of Nottingham) and Catherine Heymans (University of British Columbia)
lensed background galaxy z = 1.55 lens galaxy z = 0.168 Aragon-Salamanca et al in prep Meghan Gray (University of Nottingham) and Catherine Heymans (University of British Columbia)
Page 1 and 2: Mass, Gas and Galaxies in the Abell
Page 3 and 4: Catherine Heymans LBL 22nd Jan 2008
Page 5 and 6: The Abell 901/902 Supercluster 30x3
Page 7 and 8: QE (%) λ / nm COMBO-17 Wolf et al
Page 9 and 10: Massive ellipticals live in cluster
Page 11 and 12: Ram pressure stripping: The turbule
Page 13 and 14: 1. Galaxy-cluster gas interactions
Page 15: Seeing the invisible Meghan Gray (U
Page 19 and 20: Tangential arclets in A901a In the
Page 21 and 22: A901a In this analysis we use 60,00
Page 23 and 24: What about systematics? B E Lensing
Page 25 and 26: A901b: the most massive and X-ray r
Page 27 and 28: SW group M = 3.8 ± 0.5h −1 10 13
Page 29 and 30: Mass to stellar mass ratio Catherin
Page 31 and 32: Why Hubble? ground-based Catherine
Page 33 and 34: Future telescopes in space: a quick
Page 35 and 36: STAGES: Space Telescope A901/902 Ga
Page 37 and 38: Anatomy of a supercluster: a comple
Page 39 and 40: hidden supermassive black hole Step
Page 41 and 42: Blue Galaxies Step 3: connect galax
Page 43 and 44: What causes galaxy evolution in den

Mass, Gas and Galaxies in the Abell 901/902 Supercluster

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